FSR 1167
Summary
FSR 1167 is a sparse, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It is rarely studied in the literature, with no articles listed in the last 13 years.
This object shares a significant percentage of members with at least one entry reported in the same catalogue.
Warning: contains less than 25 stars with P>0.5 estimated.
Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Froebrich et al. (2007) | 101.617 | -10.984 | – | – | – | – |
| Kharchenko et al. (2012) | 101.588 | -10.985 | – | 1.55 | -0.36 | – |
| UCC | 101.572 | -10.978 | 0.286 | -0.942 | 0.889 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.521, distance=2325, log_age=9.385 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| FSR 1166 | 56.0 | 101.54 | -10.98 | 0.26 | -0.96 | 0.92 | 73.34 | 0.03 |